Moreover, in a recent MUSE
survey of 6 DLAs at \(z \sim 3\) ,
[1]} have obtained a high detection rate of galaxies up to \(\approx 80\%\)  within 1000 km s\(^{-1}\)  of the DLAs, with impact
parameters ranging between 25 and 280 kpc.
Notably, in contrast to previous searches, the blind survey of [1]} has yielded detections of multiple galaxies also for low metallicity systems (see their figure 9), including a galaxy group associated with a metal poor DLA (\(Z/Z_{\odot } \approx - 2.33\) ). With a small but representative sample, using cosmological simulations, these authors have
been able to place constraints on the typical mass of halos that host DLAs in the range \(10^{11}-10^{12}M_{\odot }\) .
